15 Current Work: Si(Li) Detectors GAPS will use inch, 4-strip Si(Li) detectors, 2.5mm thick Fabrication scheme developed d at Columbia University; it plan to have detectors t produced by commercial company Shimadzu in Japan. Confirmed leakage current and performance with cosmic rays and X-ray source Am-241 source FWHM: Prototype single-strip 2-inch detector with guard ring and pre-amplifier Prototype 4-inch,4-strip detector (courtesy Shimadzu Corp) Currently optimizing fabrication; ramp up to trial production runs in early 2018

Measurement of the cosmic ray positron spectrum with the Fermi LAT using the Earth s magnetic field Justin Vandenbroucke (KIPAC, Stanford / SLAC) for the Fermi LAT collaboration International Cosmic Ray

SEARCHES FOR ANTIMATTER DIETRICH MÜLLER University of Chicago SLAC SUMMER INSTITUTE 2011 OUTLINE Early History Baryon Asymmetry of the Universe? Current Limits on Antimatter Nuclei from Distant Galaxies

Solar modulation with AMS Monthly Proton Flux Veronica Bindi, AMS Collaboration Physics and Astronomy Department University of Hawaii at Manoa Honolulu, Hawaii, US 1 AMS on the ISS May 19, 2011 and for

4 Antibaryons The discovery of the antiproton and other antimatter, 1955 1959 While the existence of antiparticles was established with Anderson s discovery of the positron in 1932, it was not clear in

Particle accelerators Charged particles can be accelerated by an electric field. Colliders produce head-on collisions which are much more energetic than hitting a fixed target. The center of mass energy

Search for dark matter particles in space: International experiments PAMELA and GAMMA-400 S.A.Voronov National Research Nuclear University MEPHI Moscow Lebedev Physical Institute RAS 52th session of the

Status of the Gadolinium project for Super-Kamiokande Lluís Martí Magro. Conca Specchiulla, Italy. 5 th of September, 2010. Super-Kamiokande in the past The Super-Kamiokande collaboration had many successes

Alice TPC particle identification on the way to Anti-Nuclei and exotic states INTERNATIONAL SCHOOL OF NUCLEAR PHYSICS 34th Course Probing the Extremes of Matter with Heavy Ions Erice-Sicily: 16-24 September

The MEG/MEGII and Mu3e experiments at PSI Angela Papa Paul Scherrer Institut on behalf of the MEG/MEGII and Mu3e collaborations Contents Introduction The world s most intense DC muon beam The MEG/MEGII

Chicago State University, Chicago, USA E-mail: edmundo.garcia@csu.edu On Behalf of the ALICE Collaboration The ALICE Collaboration is preparing a major detector upgrade for the second LHC long shutdown

Status of the G A M M A - 400 Project A. M. Galper Trieste, Italy, May 2013 The main scientific objective of the GAMMA-400 Project, that was defined by Nobel laureate V. L. Ginzburg, is to search for peculiarity

What is matter and how is it formed? Lesson 6: Subatomic Particles Subatomic particles refers to particles that are more "fundamental" than... Are these fundamental particles or are they made up of smaller,

32nd International Cosmic Ray Conference, Beijing 2011 Five Years of PAMELA in orbit P. Picozza on behalf of PAMELA collaboration 1,2;1) 1 University of Rome Tor Vergata, Department of Physics, I-00133,

MEASUREMENT AND DETECTION OF RADIATION Second Edition Nicholas Tsoulfanidis University of Missouri-Rolla Ж Taylor &Francis * Publishers since I79H CONTENTS Preface to the First Edition Preface to the Second

Chapter 22 Back to the Beginning of Time Expansion of Universe implies dense, hot start: Big Bang Back to the Big Bang The early Universe was both dense and hot. Equivalent mass density of radiation (E=mc

Physics 557 Lecture 7 A brief history of accelerators, detectors and experiments: (See Chapter 14 and Appendix H in Rolnick.) First came the study of the debris from cosmic rays (the God-given particle

Collaborazione DAMA & INR-Kiev http://people.roma2.infn.it/dama XCVIII Congresso SIF Napoli, 18 Settembre 2012 F. Cappella Based on the study of the correlation between the Earth motion in the galactic